In Problems 79-84, use the following discussion. The formula D = 24 [ 1 − cos − 1 ( tan i tan θ ) π ] can be used to approximate the number of hours of daylight D when the declination of the Sun is i ∘ at a location θ ∘ north latitude for any date between the vernal equinox and autumnal equinox. The declination of the Sun is defined as the angle i between the equatorial plane and any ray of light from the Sun. The latitude of a location is the angle θ between the Equator and the location on the surface of Earth, with the vertex of the angle located at the center of Earth. See the figure. To use the formula, cos − 1 ( tan i tan θ ) must be expressed in radians. Approximate the number of hours of daylight in Anchorage, Alaska ( 61 ∘ 10 ' north latitude), for the following dates: (a) Summer solstice ( i = 23.5 ∘ ) (b) Vernal equinox ( i = 0 ∘ ) (c) July 4 ( i = 22 ∘ 48 ' )
In Problems 79-84, use the following discussion. The formula D = 24 [ 1 − cos − 1 ( tan i tan θ ) π ] can be used to approximate the number of hours of daylight D when the declination of the Sun is i ∘ at a location θ ∘ north latitude for any date between the vernal equinox and autumnal equinox. The declination of the Sun is defined as the angle i between the equatorial plane and any ray of light from the Sun. The latitude of a location is the angle θ between the Equator and the location on the surface of Earth, with the vertex of the angle located at the center of Earth. See the figure. To use the formula, cos − 1 ( tan i tan θ ) must be expressed in radians. Approximate the number of hours of daylight in Anchorage, Alaska ( 61 ∘ 10 ' north latitude), for the following dates: (a) Summer solstice ( i = 23.5 ∘ ) (b) Vernal equinox ( i = 0 ∘ ) (c) July 4 ( i = 22 ∘ 48 ' )
Solution Summary: The author calculates the number of hours of daylight D at the location north latitude.
In Problems 79-84, use the following discussion. The formula
can be used to approximate the number of hours of daylight D when the declination of the Sun is
at a location
north latitude for any date between the vernal equinox and autumnal equinox. The declination of the Sun is defined as the angle i between the equatorial plane and any ray of light from the Sun. The latitude of a location is the angle
between the Equator and the location on the surface of Earth, with the vertex of the angle located at the center of Earth. See the figure. To use the formula,
must be expressed in radians.
Approximate the number of hours of daylight in Anchorage, Alaska (
north latitude), for the following dates:
a
->
f(x) = f(x) = [x] show that whether f is continuous function or not(by using theorem)
Muslim_maths
Use Green's Theorem to evaluate F. dr, where
F = (√+4y, 2x + √√)
and C consists of the arc of the curve y = 4x - x² from (0,0) to (4,0) and the line segment from (4,0) to
(0,0).
Evaluate
F. dr where F(x, y, z) = (2yz cos(xyz), 2xzcos(xyz), 2xy cos(xyz)) and C is the line
π 1
1
segment starting at the point (8,
'
and ending at the point (3,
2
3'6
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